HR 3159
| Observation data Epoch J2000.00 Equinox J2000.00 | |
|---|---|
| Constellation | Carina[1] |
| Right ascension | 08h 00m 19.96579s[2] |
| Declination | −63° 34′ 02.8274″[2] |
| Apparent magnitude (V) | 4.81[1] |
| Characteristics | |
| Evolutionary stage | main sequence[2] |
| Spectral type | B4V[3] |
| B−V color index | −0.173±0.007[1] |
| Astrometry | |
| Radial velocity (Rv) | +22.1±2.8[1] km/s |
| Proper motion (μ) | RA: −1.762[2] mas/yr Dec.: +19.905[2] mas/yr |
| Parallax (π) | 6.9936±0.0826 mas[2] |
| Distance | 466 ± 6 ly (143 ± 2 pc) |
| Absolute magnitude (MV) | −1.11[1] |
| Details | |
| Mass | 6.3±0.1[4] M☉ |
| Radius | 3.77±0.27[5] R☉ |
| Luminosity | 912[6] L☉ |
| Surface gravity (log g) | 4.03±0.05[5] cgs |
| Temperature | 16,983[6] K |
| Metallicity [Fe/H] | −0.09±0.06[7] dex |
| Rotational velocity (v sin i) | 43[6] km/s |
| Age | 17.2±1.3[4] or 176[8] Myr |
| Other designations | |
| D Car, CD−63°866, FK5 2624, GC 10893, HD 66591, HIP 39138, HR 3159, SAO 250069[9] | |
| Database references | |
| SIMBAD | data |
HR 3159 is a single[10] star in the southern constellation of Carina, positioned near the southern constellation border with Volans. It has the Bayer designation D Carinae; HR 3159 is the Bright Star Catalogue designation. This object has a blue-white hue and is visible to the naked eye with an apparent visual magnitude of +4.81.[1] It is located at a distance of approximately 466 light years from the Sun based on parallax, and is drifting further away with a radial velocity of 22 km/s.
This object is a B-type main-sequence star with a stellar classification of B4V,[3] which indicates it is undergoing core hydrogen fusion. The star has a radius of nearly four times the radius of the Sun,[5] and over six[4] times the Sun's mass. Age estimates range from 17[4] up to 176[8] million years old, and it is spinning with a projected rotational velocity of 43 km/s.[6] It is radiating 912[6] times the luminosity of the Sun from its photosphere at an effective temperature of 16,983 K.[6]
References
- ^ a b c d e f Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015, S2CID 119257644.
- ^ a b c d e f Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ a b Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1975mcts.book.....H.
- ^ a b c d Tetzlaff, N.; et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv:1007.4883, Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966.2010.17434.x, S2CID 118629873.
- ^ a b c Fitzpatrick, E. L.; Massa, D. (March 2005), "Determining the Physical Properties of the B Stars. II. Calibration of Synthetic Photometry", The Astronomical Journal, 129 (3): 1642–1662, arXiv:astro-ph/0412542, Bibcode:2005AJ....129.1642F, doi:10.1086/427855, S2CID 119512018.
- ^ a b c d e f Balona, L. A.; et al. (May 2019), "Rotational modulation in TESS B stars", Monthly Notices of the Royal Astronomical Society, 485 (3): 3457–3469, arXiv:1902.09470, Bibcode:2019MNRAS.485.3457B, doi:10.1093/mnras/stz586.
- ^ Gáspár, András; et al. (2016), "The Correlation between Metallicity and Debris Disk Mass", The Astrophysical Journal, 826 (2): 171, arXiv:1604.07403, Bibcode:2016ApJ...826..171G, doi:10.3847/0004-637X/826/2/171, S2CID 119241004.
- ^ a b Gontcharov, G. A. (November 2012), "Spatial distribution and kinematics of OB stars", Astronomy Letters, 38 (11): 694–706, arXiv:1606.09028, Bibcode:2012AstL...38..694G, doi:10.1134/S1063773712110035, S2CID 119108982.
- ^ "HD 66591". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-12-04.
- ^ Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.